Physics
Scientific paper
Feb 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007phrvc..75b5802b&link_type=abstract
Physical Review C, vol. 75, Issue 2, id. 025802
Physics
14
Nuclear Matter Aspects Of Neutron Stars, Nuclear Matter, Many-Body Theory
Scientific paper
We studied the influence of dispersive self-energy effects, three-body forces, and polarization contributions to the interaction kernel on the 1S0 proton pairing in neutron star matter. We found that a strong suppression of the gap by self-energy effects and three-body forces is at low density compensated by the attractive polarization interaction, shifting the domain of pairing to below ρB≈0.3fm-3.
Baldo Marcello
Schulze Hans-Josef
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